The observed galaxy presents a generally smooth morphology, exhibiting a primarily elliptical shape. There is an absence of clearly defined spiral arms or a prominent central bulge. The galaxy appears to be moderately elongated, tending toward a cigar-shaped form. There is no obvious evidence of ongoing major merger activity or significant tidal disturbances, though a possible minor disturbance cannot be ruled out. The light distribution is relatively uniform, with a concentration of luminosity towards the core. The overall color suggests a mix of stellar populations, with a slight redder hue implying a potentially higher fraction of older stars. The galaxy's size appears to be relatively moderate. Star formation appears present, though not at an extreme rate.
