The galaxy presents a generally smooth and rounded morphology, with a concentrated central bulge. The color profile suggests a population of older stars, particularly in the bulge region where a yellowish hue dominates. There is some evidence of a faint, extended disk structure surrounding the bulge, exhibiting a slightly bluer color, possibly indicating some ongoing, albeit low-level, star formation. No strong spiral arms or significant dust lanes are discernible. The overall appearance suggests an intermediate morphological type, potentially an early-type spiral or a lenticular galaxy. There is no obvious indication of any major ongoing merger activity or significant tidal disturbances.
