The galaxy presents a generally smooth, elliptical morphology. The central region displays a concentrated luminosity, indicating a dense stellar population or potentially an active galactic nucleus. The galaxy exhibits a slight elongation, deviating marginally from a perfectly circular form. There is an apparent lack of distinct spiral arm structures or prominent dust lanes. The color profile transitions from a yellowish-white core to slightly bluer hues in the outer regions, suggestive of ongoing, albeit potentially subdued, star formation. There is no obvious evidence of any major interaction or merging event, although subtle disturbances cannot be entirely ruled out at this resolution. The overall appearance points towards a relatively evolved system, possibly transitioning towards a lenticular or early-type spiral classification.
