The galaxy presents a generally smooth morphology. Its overall shape is elongated, appearing cigar-shaped, with an estimated effective radius of around 16 kpc. The central region exhibits a concentrated luminosity, suggesting a prominent bulge. The galaxy's color profile indicates a relatively redder hue, possibly implying a population of older stars, although there is evidence of moderate star formation occurring. There are subtle signs of minor disturbances in its structure, with potential interactions or tidal features. The overall impression is that of a mature galaxy undergoing some degree of ongoing evolution.
