The galaxy presents an elliptical morphology with a high degree of central concentration. The light distribution appears smooth and lacks any distinct spiral arm structures or prominent dust lanes. The overall color profile suggests the presence of a mixed stellar population. The central region exhibits a brighter, slightly redder hue, possibly indicating a higher concentration of older stars. The outer regions show a subtle shift toward bluer tones, perhaps suggesting some ongoing or recent star formation activity, even if it is minimal. The galaxy's shape is elongated, showing a cigar shape in the distribution of starlight. There are indications of minor disturbances that might be a merging process or interactions with other galaxies. The overall impression is that of a relatively massive galaxy with a complex evolutionary history.
