The galaxy presents as a relatively small, elongated object with a high degree of asymmetry. Its morphology is suggestive of a late-type spiral or an irregular galaxy viewed edge-on. The central bulge is not prominent, and the light distribution indicates a more uniform stellar population throughout the disk. There is no clear evidence of tightly wound spiral arms, but subtle variations in color suggest possible faint structures within the galaxy disk. The overall color profile shows a subtle shift toward redder hues, possibly indicating a population of older stars or dust obscuration. Evidence of active star formation is limited, with no prominent HII regions or bright knots visible within the galaxy's disk. There is no evidence of strong tidal features or interactions with other galaxies in the immediate vicinity. The lack of significant morphological disturbances suggests a relatively isolated system that is not currently undergoing major merger activity, although the galaxy's lopsided shape is suggestive of a past or ongoing minor interaction.
