The galaxy presents as a slightly elongated, cigar-shaped structure. It displays a relatively smooth morphology, with no immediately apparent spiral arms or distinct features indicative of active star formation regions. The color profile suggests a population dominated by older stars, emitting predominantly in the redder wavelengths, with diminishing blue light from younger stars. There's no obvious dust lane or signs of major disturbances, tidal tails, or merging activity, although a possible minor disturbance is not out of the question. Overall, this galaxy appears to be an evolved system with a sizable stellar mass and relatively low ongoing star formation activity.
